Berkeley 54

(MWSC 3456; OCL 194; FSR 0256)

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C3
N_50
r_50
AB 544 1.6
Summary

Berkeley 54 is a very rich, very dense object of high C3 quality. It is located at a large distance from the Sun, below the mid-plane. It is well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 315.8 40.467 -1.87 -5.43
Kharchenko et al. (2013) 315.75 40.44 -2.66 -0.82
Kharchenko et al. (2016) 315.745 40.437
Loktin & Popova (2017) 315.75 40.437 -0.138 -0.181
Cantat-Gaudin et al. (2018) 315.745 40.433 0.12 -3.091 -3.254
Bica et al. (2019) 315.789 40.462
Soubiran et al. (2018) 315.745 40.433 -56.21
Cantat-Gaudin et al. (2020) 315.745 40.433 0.12 -3.091 -3.254
Dias et al. (2021) 315.744 40.431 0.119 -3.086 -3.256 -54.951
Just et al. (2023) 315.745 40.437
Hunt & Reffert (2023) 315.742 40.429 0.149 -3.075 -3.308 -48.879
Cavallo et al. (2024) 315.737 40.429 0.14
Hunt & Reffert (2024) 315.742 40.429 0.149 -3.075 -3.308 -48.879
Almeida et al. (2025) 315.744 40.431
Hu & Soubiran (2025) 315.737 40.429
           
UCC 315.744 40.433 0.138 -3.105 -3.288 -55.072
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.77, Dist=2300.0, Age=9.6
Kharchenko et al. (2013) E(B-V)=1.135, d=4236.0, logt=8.985
Kharchenko et al. (2016) E(B-V)=1.135, d=4236.0, logt=8.985
Loktin & Popova (2017) E(B-V)=1.021, Dist=2233, logt=9.34
Cantat-Gaudin et al. (2018) dmode=6706.0
Soubiran et al. (2018) dmode=6706.0
Cantat-Gaudin et al. (2020) AVNN=2.24, DistPc=6680.0, AgeNN=9.43
Dias et al. (2021) Av=2.623, Dist=6955, logage=9.277, [Fe/H]=0.029
Just et al. (2023) logt=8.985, logmt=2.932
Hunt & Reffert (2023) AV50=3.226, diffAV50=2.058, MOD50=13.748, logAge50=8.895
Cavallo et al. (2024) AV50=2.66, dMod50=14.06, logAge50=9.34, [Fe/H]50=-0.31
Hunt & Reffert (2024) MassJ=3086.79, MassTot=3478.21
Almeida et al. (2025) AV=2.623, Dist=6955, logAge=9.277, MassRk=6146.7
Hu & Soubiran (2025) MA22=-0.19, MA23f=-0.2, MA23g=-0.13, MZ23=-0.23, MK24=-0.21, MF24=-0.13

Search coordinates in Bayestar19

Cluster region map